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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.3390/sym11111401</dc:identifier><dc:language>eng</dc:language><dc:creator>Carmona, José Manuel</dc:creator><dc:creator>Cortés, José Luis</dc:creator><dc:creator>Relancio, José Javier</dc:creator><dc:title>Spacetime and deformations of special relativistic kinematics</dc:title><dc:identifier>ART-2019-115874</dc:identifier><dc:description>A deformation of special relativistic kinematics (possible signal of a theory of quantum gravity at low energies) leads to a modification of the notion of spacetime. At the classical level, this modification is required when one considers a model including single- or multi-interaction processes, for which absolute locality in terms of canonical spacetime coordinates is lost. We discuss the different alternatives for observable effects in the propagation of a particle over very large distances that emerge from the new notion of spacetime. A central ingredient in the discussion is the cluster decomposition principle, which can be used to favor some alternatives over the others.</dc:description><dc:date>2019</dc:date><dc:source>http://zaguan.unizar.es/record/87747</dc:source><dc:doi>10.3390/sym11111401</dc:doi><dc:identifier>http://zaguan.unizar.es/record/87747</dc:identifier><dc:identifier>oai:zaguan.unizar.es:87747</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/DGIID-DGA/2015-E24-2</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO-FEDER/PGC2018-095328-B-I00</dc:relation><dc:identifier.citation>Symmetry 11, 11 (2019), 1401  [13 pp.]</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>http://creativecommons.org/licenses/by/3.0/es/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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